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Table 3.

Background galaxies in the MUSE field.

MSB α (J2000) δ (J2000) Vo Io z Diagnostic
19 10 21 42.43 +18 05 17.38 23.41 21.70 0.5436 [O II] λ3727
39 10 21 42.46 +18 05 42.80 23.88 22.33 0.7543 [O II] λ3727
56 10 21 42.55 +18 05 47.16 24.62 22.53 0.5169 [O II] λ3727
37 10 21 42.56 +18 05 17.56 24.19 22.24 0.7554 [O II] λ3727
4 10 21 42.62 +18 05 14.59 21.95 20.26 0.3925 Ca H + K
62 10 21 42.87 +18 05 33.13 24.15 22.64 0.7539 [O II] λ3727
48 10 21 42.97 +18 05 38.43 24.22 22.40 0.7549 [O II] λ3727
30 10 21 42.99 +18 05 08.98 23.30 22.62 2.5007 Near-UV Fe II, Mg II
49 10 21 43.01 +18 05 59.13 23.98 22.50 0.8883 [O II] λ3727
26 10 21 43.04 +18 05 08.34 23.29 22.36 2.5005 Near-UV Fe II, Mg II
7 10 21 43.10 +18 05 17.26 23.07 20.88 0.5440 [O II] λ3727
31 10 21 43.39 +18 05 38.07 23.60 22.25 0.7462 [O II] λ3727
17 10 21 44.15 +18 05 03.11 22.84 21.82 0.4763 [O II] λ3727
108 10 21 44.15 +18 05 11.12 24.29 23.23 0.8320 [O II] λ3727
10 21 44.44 +18 05 05.53 ... ... 0.4763 [O II] λ3727
168 10 21 45.28 +18 05 34.77 24.57 24.17 0.3603 [O II] λ3727
151 10 21 45.68 +18 05 38.30 25.00 23.38 0.6028 [O II] λ3727
172 10 21 46.04 +18 05 35.46 24.78 23.67 0.8149 [O II] λ3727
163 10 21 46.05 +18 05 49.46 24.86 23.52 0.9692 [O II] λ3727
10 21 46.18 +18 05 59.60 ... ... 0.4137 Ca H + K

Notes.

Identifiers and magnitudes are from McQuinn et al. (2013). MSB 56 was previously identified as a candidate C-AGB star by Lee (2016). Typical uncertainties on the estimated redshifts are ±0.0002, except for #26 and 30, where the dispersion of the seven near-UV lines (Fe II λ λ2343, 2374, 2382, 2586, 2599; Mg II λ λ2796, 2803) was ±0.0005.

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